Orion Sirius EQ?G User manual

Brand: Orion

Model: Sirius EQ?G

Category: Telescopes

Type: User manual

This manual is also suitable for

sirius 9995

INSTRUCTION MANUAL

IN 280 Rev. B 02/06

Providing Exceptional Consumer Optical Products Since 1975

Customer Support (800)-676-1343

E-mail: [email protected]

Corporate Offices (831)‑763‑7000

89 Hangar Way, Watsonville, CA 95076

Orion® Sirius™ EQ-G

Equatorial Mount

#9995

Figure 1. The Sirius EQ-G mount.

Tube ring mounting plate

Declination lock lever (not shown)

Front opening

Declination setting circle

Counterweight shaft lock lever

Counterweight lock knob

Counterweight

Counterweight shaft

“Toe-saver”

Tripod center support tray

Tripod leg

Mounting plate lock knobs

Control panel

Right ascension lock lever

Right ascension setting circle

Latitude scale

Latitude adjustment L-bolts

Hand controller cable

Center support shaft

GoTo hand controller

Leg lock levers

Table of Contents

1. Unpacking............................ 3

2. Parts List............................. 3

3. Assembly ............................ 3

4. Attaching a Telescope................... 4

5. Balancing a Telescope .................. 4

6. Setting Up and Using the Equatorial Mount . . 5

7. The Sirius EQ-G Dual-Axis Hand Controller.. 8

8. The Sirius EQ-G GoTo Hand Controller .... 10

9. Specifications ........................ 20

10. Appendices ......................... 21

1. Unpacking

The entire mount will arrive in three boxes, one containing

the tripod, one containing the equatorial mount and one con-

taining the hand controller. Be careful unpacking the boxes.

We recommend keeping the boxes and original packaging.

In the event that the mount needs to be shipped to another

location, or returned to Orion for warranty repair, having the

proper packaging will ensure that your mount will survive the

journey intact.

Make sure all the parts in the Parts List are present. Be

sure to check the box carefully, as some parts are small.

If anything appears to be missing or broken, immediate-

ly call Orion Customer Support (800-676-1343) or email

suppor[email protected] for assistance.

2. Parts List

Box 1: Tripod

Qty. Item

1 Tripod

1 Counterweight (11lbs.)

1 Tripod center support tray

Box 2: Equatorial Mount

Qty. Item

1 Equatorial mount

1 Tube ring mounting plate

1 12V DC Power cable

If you’ve purchased the #7944 Dual-Axis hand controller:

Box 3: Dual-Axis Hand Controller

Qty. Item

1 Dual-Axis hand controller

2 Nylon hook-and-loop strips (1 hook strip, 1 loop

strip)

1 Wire clip

If you’ve purchased the #7947 GoTo hand controller:

Box 3: GoTo Hand Controller

Qty. Item

1 GoTo hand controller

1 GoTo hand controller cable for Sirius EQ-G

1 GoTo hand controller cable for Atlas EQ-G

1 GoTo hand controller bracket

1 Computer interface cable (RS-232)

1 Wire clip

3. Assembly

Refer to Figure 1 as needed during the assembly process.

1. Stand the tripod legs upright and spread the legs out as

far as they will go. Make certain that the leg lock levers

are tightened. Keep the tripod legs at their shortest (fully

retracted) length, for now; you can extend them to a more

desirable length later, after the mount is fully assembled.

2. Place the base of the equatorial mount onto the tripod

head. Orient the equatorial mount so that the post on the

tripod head lines up with the azimuth adjustment knobs on

the equatorial mount (Figure 2). You may need to loosen

Congratulations on your purchase of a quality Orion mount. Your new Sirius EQ-G mount works with many different

optical tubes. Designed for astronomical use, the Sirius EQ-G provides a solid, stable foundation for precise navigation of the

night sky. The internally-housed, dual-axis stepper motors provide smooth slewing and tracking of any celestial object. With a

little practice, you’ll find that the Sirius EQ-G mount is an invaluable tool for getting the most out of your astronomical observing

sessions.

These instructions will help you set up and properly use your equatorial mount. Please read them over thoroughly before getting

started.

Figure 2. Orient the equatorial head so the post on the tripod

lines up with the azimuth adjustment knobs on the equatorial mount.

Azimuth

adjustment

knobs

Post

the azimuth adjustment knobs on the equatorial mount in

order to fit the mount onto the tripod head.

3. Thread the central support shaft up through the tripod

head and into the bottom of the equatorial mount until

tight. Use the upper knob on the central support shaft to

do this. The equatorial mount should now be firmly con-

nected to the tripod.

4. Remove the knob and washer from the bottom of the

center support shaft. Slide the tripod support tray up the

bottom of the central support shaft until the three tray

arms are touching the legs of the tripod. The flat side of

the support tray should be facing up. Make sure the “V” of

each tray arm is against a tripod leg. Place the washer on

the center support shaft against the tray, and follow it by

threading the knob all the way up the center support shaft

until it is tight against the tray. The tripod support tray pro-

vides additional stability for the tripod, and holds up to five

1.25" eyepieces and two 2" eyepieces.

5. Loosen the counterweight shaft lock lever and fully extend

the counterweight shaft. Retighten the lock lever.

6. Remove the knurled “toe saver” retaining screw on the bot-

tom of the counterweight shaft and slide the counterweight

onto the shaft. Make sure the counterweight lock knob is

adequately loosened to allow the counterweight shaft to

pass through the hole. Position the counterweight about

halfway up the shaft and tighten the lock knob. Replace

the toe saver at the end of the bar. The toe saver prevents

the counterweight from falling on your foot if the lock knob

happens to come loose.

Your Sirius EQ-G mount is now fully assembled and should

resemble Figure 1 except for the hand controller, which will

be installed and explained in Section 7 (Dual-Axis) or Section

8 (GoTo).

4. Attaching a Telescope

The Sirius EQ-G equatorial mount is designed to hold tele-

scope tubes weighing up to approximately 25 lbs. For heavier

telescopes, the mount may not provide sufficient stability for

steady imaging. Any type of telescope can be mounted on the

Sirius EQ-G, including refractors, Newtonian reflectors, and

catadiotropics, provided a set of tube rings is available to cou-

ple the tube to the mount. Orion sells a variety of telescope

tube rings. Please visit our website at OrionTelescopes.com

for details.

1. Attach the tube mounting rings to the tube ring mounting

plate using the screws that come with the tube rings. The

screws should go through the center holes in the ends of

the mounting plate and rethread into the tube rings. Note

that the side of the mounting plate with the central “groove”

will be facing up (Figure 3). Use a small wrench to secure

the tube rings to the mounting plate.

Note: The tube ring mounting plate included with the Sirius

EQ-G includes four optical axis offset adjustment screws;

these are the socket head cap screws located at each cor-

ner of the mounting plate. These adjustment screws will be

explained further in Appendix A. For now, confirm that all four

adjustment screws are sufficiently unthreaded so that the

ends of their threaded shafts are flush with the top surface of

the tube ring mounting plate.

Note: The optical axis offset adjustment screws should be

oriented so that the threaded shaft extends upward through

the top surface of the tube ring mounting plate. If the tube

ring mounting plate arrives with the optical axis offset screws

installed backwards, reverse their orientation before proceed-

ing (Figure 3).

2. Loosen the black mounting plate lock knobs on the top of

the equatorial mount. Place the mounting plate, with the

tube rings attached, in the slot on top of the equatorial

mount. Position the mounting plate so that it is centered in

the slot. Re-tighten the mounting plate lock knobs until the

plate is secure.

3. Open the tube rings by unthreading the knurled clamps

and lay the telescope optical tube in the rings at about

the midpoint of the tube’s length. Rotate the tube so that

the focuser is at a convenient height for viewing. Close the

tube rings and retighten the clamps.

Note: Some telescope optical tubes (specifically Schmidt-

Cassegrains and Maksutov-Cassegrains) have a mounting

plate connected directly to the tube. For these telescopes,

optional tube rings are not required. Simply follow step 2

(above) to connect the telescope to the mount.

5. Balancing a Telescope

To ensure smooth movement of a telescope on both axes of

the equatorial mount, it is imperative that the optical tube is

properly balanced. We will first balance the telescope with

respect to the right ascension (R.A.) axis, then the declination

(Dec.) axis.

1. Keeping one hand on the telescope optical tube, loosen

the R.A. lock lever. Make sure the Dec. lock lever is locked,

for now. The telescope should now be able to rotate freely

about the right ascension axis. Rotate it until the counter-

weight shaft is parallel to the ground (i.e., horizontal).

2. Now loosen the counterweight lock knob and slide the

weight along the shaft until it counterbalances the tele-

scope (Figure 4a). That’s the point at which the shaft

remains horizontal even when you let go with both hands

(Figure 4b). If the telescope refuses to balance then you

Figure 3. The tube ring mounting plate.

Optical axis offset

adjustment screws

Flat washer

Lock washer

Tube ring

attachment screw

have either too much or too little counterweight. Remove

counterweight, or add optional counterweights if needed.

3. Retighten the counterweight lock knob. The telescope is

now balanced on the right ascension axis.

4. To balance the telescope on the declination axis, first tight-

en the R.A. lock lever, with the counterweight shaft still in

the horizontal position.

5. With one hand on the telescope optical tube, loosen the

Dec. lock lever. The telescope should now be able to rotate

freely about the declination axis.

6. Loosen the knurled ring clamps on the tube rings a few

turns, until you can slide the telescope tube forward and

back inside the rings (this can be aided by using a slight

twisting motion on the optical tube while you push or pull

on it) (Figure 4c). If the mounting plate is connected directly

to your telescope’s tube (i.e. tube rings are not utilized), you

can balance the telescope in Dec. by sliding the mounting

plate forward or back in the slot on top of the equatorial

mount.

7. Position the telescope in the tube rings so it remains hori-

zontal when you carefully let go with both hands. This is the

balance point for the optical tube with respect to the Dec.

axis (Figure 4d).

8. Retighten the knurled ring clamps.

The telescope is now balanced on both axes. When you loos-

en the lock lever on one or both axes and manually point the

telescope, it should move without resistance and should not

drift from where you point it.

6. Setting Up and Using the

Equatorial Mount

When you look at the night sky, you no doubt have noticed

that the stars appear to move slowly from east to west over

time. That apparent motion is caused by the Earth’s rotation

(from west to east). An equatorial mount (Figure 5) is designed

to compensate for that motion, allowing you to easily “track”

the movement of astronomical objects, thereby keeping them

from drifting out of your telescope’s field of view while you’re

observing.

This is accomplished by slowly rotating the telescope on its

right ascension (R.A.) axis, using the built in motor drive. But

first the R.A. axis of the mount must be aligned with the Earth’s

rotational (polar) axis—a process called polar alignment.

Polar Alignment

For Northern Hemisphere observers, approximate polar align-

ment is achieved by pointing the mount’s right ascension axis

at the North Star, or Polaris. It lies within 1° of the north celes-

tial pole (NCP), which is an extension of the Earth’s rotational

axis out into space. Stars in the Northern Hemisphere appear

to revolve around the NCP.

Figure 6. To find Polaris in the night sky, look north and find the

Big Dipper. Extend an imaginary line from the two “Pointer Stars” in

the bowl of the Big Dipper. Go about five times the distance between

those stars and you'll reach Polaris, which lies within 1° of the north

celestial pole (NCP).

Big Dipper

(in Ursa Major)

Little Dipper

(in Ursa Minor)

Cassiopeia

N.C.P.

Pointer

Stars

Polaris

Figure 5. The Sirius EQ-G mount.

Polar axis finder scope

Latitude scale

Latitude adjustment

L-bolts

Dec lock lever

Front opening

Right

Ascension

(R.A.) axis

R.A. lock lever

Declination (Dec) axis

Figure 4a-d. Proper operation of the equatorial mount requires

that the telescope tube be balanced on the R.A. and Dec. axes. (a)

With the R.A. lock lever released, slide the counterweight down the

counterweight shaft until it just counterbalances the telescope tube.

(b) When you let go with both hands, the tube should not drift up or

down. (c) With the Dec. lock lever released, loosen the tube ring lock

clamps a few turns and slide the telescope forward or back in the

tube rings. (d) When the tube is balanced about the Dec. axis, it will

not move when you let go.

a. b.

c. d.

To find Polaris in the sky, look north and locate the pattern of

the Big Dipper (Figure 6). The two stars at the end of the “bowl”

of the Big Dipper point right to Polaris.

Observers in the Southern Hemisphere aren’t so fortunate to

have a bright star so near the south celestial pole (SCP). The

star Sigma Octantis lies about 1° from the SCP, but it is barely

visible with the naked eye (magnitude 5.5).

For general visual observation, an approximate polar align-

ment is sufficient.

1. Level the equatorial mount by adjusting the length of the

three tripod legs.

2. There are two latitude adjustment L-bolts (see Figure 5);

loosen one while tightening the other. By doing this you

will adjust the latitude of the mount. Continue adjusting the

mount until the pointer on the latitude scale is set at the

latitude of your observing site. If you don’t know your lati-

tude, consult a geographical atlas to find it. For example, if

your latitude is 35° North, set the pointer to 35. The latitude

setting should not have to be adjusted again unless you

move to a different viewing location some distance away.

3. Loosen the Dec. lock lever and rotate the telescope’s opti-

cal tube until it is parallel with the right ascension axis, as it

is in Figure 5.

4. Move the tripod so the telescope tube and right ascen-

sion axis point roughly at Polaris. If you cannot see Polaris

directly from your observing site, consult a compass and

rotate the tripod so the telescope points north.

The equatorial mount is now polar aligned for casual observing.

More precise polar alignment is recommended for astropho-

tography. For this we recommend using the polar axis finder

scope.

From this point on in your observing session, you should not

make any further adjustments to the latitude of the mount, nor

should you move the tripod. Doing so will undo the polar align-

ment. The telescope should be moved only about its R.A. and

Dec. axes.

The Polar Axis Finder Scope

The Sirius EQ-G mount comes with a polar axis finder scope

(Figure 7) housed inside the right ascension axis of the mount.

When properly aligned and used, it makes accurate polar

alignment quick and easy to do. Unthread the cover at the rear

of the mount’s right ascension axis and remove the cap on

the front opening of the equatorial mount (Figure 5) to view

through the polar axis finder scope.

Alignment of the Polar Axis Finder Scope

1. Loosen the Dec. lock lever and rotate the optical tube on

the declination axis until you have a clear view through the

polar axis finder scope (Figure 8). Tighten the Dec. lock

lever.

2. Look through the polar finder at a distant object (during the

day) and center it in the crosshairs. You may need to adjust

the latitude adjustment L-bolts and the tripod position to do

this. Focus the polar finder by rotating the eyepiece.

3. Rotate the mount 180° about the R.A. axis. It may be con-

venient to remove the counterweights and optical tube

before doing this.

4. Look through the polar finder again. Is the object being

viewed still centered on the crosshairs? If it is, then no fur-

ther adjustment is necessary. If not, then look through the

polar finder while rotating the mount about the R.A. axis.

You will notice that the object you have previously centered

moves in a circular path. Use the three alignment set-

screws on the polar axis finder (Figure 7) to redirect the

crosshairs of the polar finder to the apparent center of this

circular path.

5. Repeat this procedure until the position the crosshairs point

to does not rotate off-center when the mount is rotated in

R.A.

The polar axis finder scope is now ready to be used. When not

in use, replace the plastic protective cover to prevent the polar

finder from getting bumped.

Figure 7. The polar axis finder scope.

Eyepiece

focus ring

Alignment

setscrew (3)

Focus

lock ring

Objective

lens

Figure 8. The optical tube must be rotated about the Dec. axis

until you have a clear view along the R.A. axis with the polar axis

finder scope.

Objective lens

of polar axis

finder scope

Using the Polar Axis Finder Scope

The reticle of the polar axis finder scope for the Sirius EQ-G

has a tiny star map printed on it that makes precise polar align-

ment quick and easy. To polar align the mount using the polar

axis finder scope, follow these instructions:

1. Approximately polar-align the mount as outlined in the pro-

cedure above.

2. Loosen the Dec. lock lever and rotate the optical tube on

the declination axis until you have a clear view through

the polar axis finder scope along the right ascension axis

(Figure 8). Tighten the Dec. lock lever.

3. Focus the polar finder by rotating the eyepiece. Now, sight

Polaris in the polar axis finder scope. If you have followed

the approximate polar alignment procedure accurately,

Polaris will probably be within the field of view. If not, move

the tripod left-to-right, and adjust the latitude up-and down

until Polaris is somewhere within the field of view of the

polar axis finder scope.

Note: If you do not have a clear view of Polaris from your

observing site, you will not be able to use the polar axis finder

to precisely polar align the telescope.

4. The mount has a built-in illuminator that allows you to see

the reticle pattern in the polar axis finder scope at night.

Simply turn on the power switch on the Sirius EQ-G mount

(see “Powering the Sirius EQ-G Mount”) and the polar axis

finder scope reticle will be illuminated. Note the constel-

lation Cassiopeia and the Big Dipper in the reticle. They

do not appear in scale, but they indicate the general posi-

tions of Cassiopeia and the Big Dipper relative to the North

Celestial Pole (which is indicated by the cross at the cen-

ter of the reticle). Rotate the reticle so the constellations

depicted match their current orientation in the sky when

viewed with the naked eye. To do this, release the R.A. lock

lever and rotate the main telescope around the R.A. axis

until the reticle is oriented with sky. For larger optical tubes,

you may need to remove the tube from the mount to pre-

vent it from bumping into the mount. Once the reticle is cor-

rectly oriented, use the right ascension lock lever to secure

the mount’s position.

5. Now use the azimuth adjustment knobs (Figure 2) and the

latitude adjustment L-bolts (Figure 5) on the mount to posi-

tion the star Polaris inside the tiny circle marked “Polaris”

on the finder’s reticle. You must first loosen the knob under-

neath the equatorial mount on the center support shaft to

use the azimuth adjustment knobs. Once Polaris is properly

positioned within the reticle, you are precisely polar aligned.

Retighten the knob underneath the equatorial mount.

From this point on in your observing session, you should not

make any further adjustments in the azimuth or the latitude

of the mount, nor should you move the tripod. Doing so will

undo the polar alignment. The telescope should be moved only

about its right ascension and declination axes.

Additional Note Regarding Focusing the Polar Axis Finder

Scope

The polar axis finder scope is normally focused by simple rota-

tion of the eyepiece focus ring. However, if after adjusting the

focus ring you find that the image of the reticle is sharp, but

the stars are out of focus, then you must adjust the focus of

the polar axis finder’s objective lens. To do this, first remove

the polar axis finder from the mount by unthreading it. Look

through the polar axis finder at a star (at night) or distant object

at least 1/4 mile away (during daylight). Use the eyepiece focus

ring to bring the reticle into sharp focus. Now, loosen the focus

lock ring (Figure 7) and thread the entire objective end of the

finder inward or outward until images appear sharp. Re-tighten

the focus lock ring. Once the polar axis finder’s objective lens

is focused, it should not need to be adjusted again.

Confused About Pointing the Telescope?

Beginners occasionally experience some confusion about how

to point the telescope overhead or in other directions. In Figure

1 the telescope is pointed north as it would be during polar

alignment. The counterweight shaft is oriented downward. But

it will not look like that when the telescope is pointed in other

directions. Let’s say you want to view an object that is directly

overhead, at the zenith. How do you do it?

DO NOT make any adjustment to the latitude adjustment L-

bolts. That will spoil the mount’s polar alignment. Remember,

once the mount is polar aligned, the telescope should be

moved only on the R.A. and Dec. axes. To point the scope

overhead, first loosen the R.A. lock lever and rotate the tele-

scope on the right ascension axis until the counterweight shaft

is horizontal (parallel to the ground). Then loosen the Dec. lock

lever and rotate the telescope until it is pointing straight over-

head. The counterweight shaft is still horizontal. Then retighten

both lock levers.

What if you need to aim the telescope directly north, but at an

object that is nearer to the horizon than Polaris? You can’t do

Figure 9a-d. These illustrations show the telescope pointed in the four cardinal directions. (a) north, (b) south, (c) east, (d) west. Note

that the tripod and mount have not been moved; only the telescope has been moved on the its R.A. and Dec. axes.

a. b. c. d.

it with the counterweights down as pictured in Figure 1. Again,

you have to rotate the scope in right ascension so that the

counterweight shaft is positioned horizontally. Then rotate the

scope in declination so it points to where you want it near the

horizon.

To point the telescope directly south, the counterweight shaft

should again be horizontal. Then you simply rotate the scope

on the declination axis until it points in the south direction.

To point the telescope to the east or west, or in other directions,

you rotate the telescope on its right ascension and declina-

tion axes. Depending on the altitude of the object you want to

observe, the counterweight shaft will be oriented somewhere

between vertical and horizontal.

Figure 9 illustrates how the telescope will look when pointed

at the four cardinal directions: north (Figure 9a), south (Figure

9b), east (Figure 9c) and west (Figure 9d).

The key things to remember when pointing the telescope are

that a) you only move it in right ascension and declination, not

in azimuth or latitude (altitude), and b) the counterweight and

shaft will not always appear as it does in Figure 1. In fact it

almost never will!

7. The Sirius EQ-G Dual-Axis

Controller

The Sirius EQ-G with dual-axis hand controller will automati-

cally track any celestial object as the Earth rotates. You can

also use the controller’s directional buttons to center objects

within your telescope’s finderscope or eyepiece. For imaging

purposes, the controller provides several guide speed rates so

a camera can be accurately guided during a long exposure.

Attaching the Dual-Axis Controller

The dual-axis controller has a cable with a modular connector

on one end. Plug the modular connector into the jack on the

control panel of the mount (Figure 9.1) until it clicks into place.

The nylon hook-and-loop strips have been provided so the

dual-axis hand controller can be placed in a convenient posi-

tion on the mount when not in use. Place the “hooks” strip on

the back of the dual-axis hand controller, and the “loops” strip

on the mount in a convenient location. Make certain the loca-

tion of the strip on the mount will not cause the dual-axis hand

controller to interfere with the motions of the mount or tele-

scope.

You can reduce the chances of getting your hand controller,

power supply, or other cables tangled during use of the Sirius

EQ-G by using the included wireclip. The clip also reduces

mechanical strain on the cable. The wire clip is adhesive

backed for easy attachment to any convenient location on the

mount.

Powering the Sirius EQ-G Mount

The Sirius EQ-G should be powered by a 12V DC power supply

(tip positive) capable of producing continuous current with a mini-

mum of 2 amps. We recommend using a portable rechargeable

battery, like the Dynamo or Dynamo Pro available from Orion.

If you are using a portable battery like the Orion Dynamo, use

the supplied 12V DC power cable (male cigarette lighter plug

on one end, standard 12V DC power plug on the other end)

to connect the battery to the 12V DC power jack on the con-

trol panel of the mount (Figure 9.1). Make sure the Dynamo’s

power switch is in the “on” position after connecting.

Note: The power indicator LED on the mount (near the power

switch) will begin to flash when the battery power is low. When

the battery power is extremely low, the LED will flash rapidly.

Recharge or replace the battery as needed.

Functions of the Dual-Axis Hand Controller

There are three main categories of control buttons on the dual-

axis controller (Figure 9.2):

Figure 9.1. The Sirius EQ-G control panel.

Autoguider

jack

Power switch

Power indicator light

12V DC power

jack

Hand

controller

jack

Speed

buttons

Directional

buttons

Set button

Figure 9.2. The Sirius EQ-G Dual Axis hand controller.

1. Speed buttons

2. Directional buttons

3. Set button

The dual-axis hand controller is equipped with a red LED light

in each button to indicate operation. An individual button’s LED

will illuminate when the button is pressed. If a button combina-

tion is entered, all LEDs will illuminate to indicate a successful

operation.

Speed Buttons

The three buttons located near the top of the dual-axis hand

controller (Guide, Slow, and Fast) are used to set the slewing

and guiding speed of the mount.

Directional Buttons

The directional buttons allow complete control of the mounted

telescope’s position during slewing or tracking. The Left and

Right directional buttons control movements about the right

ascension (R.A.). axis. The Up and Down directional buttons

control movements about the declination (Dec.) axis.

Set Button

The Set button is used to set the dual-axis hand controller to

operate in either Northern or Southern hemisphere locations.

Note: The Go button is not used in normal operation of the

dual-axis controller.

Tracking Objects with the Dual-Axis Hand

Controller

In order for your Sirius EQ-G mount to accurately track celes-

tial objects as they appear to migrate across the night sky,

your mount must be properly polar aligned. For more details

on polar alignment, please consult section 6 of this manual.

Once the power switch is turned on, the dual-axis controller

begins to track by rotating the R.A. axis motor at the default

(sidereal) rate. The Dec. axis motor will not rotate. As long as

the mount has been properly polar aligned, it should not be

necessary to adjust the Dec. axis for accurate tracking. If you

notice a lack of tracking precision at the default (sidereal) rate,

consult section 6 of this manual and attempt to polar align the

mount more accurately.

Tracking can be deactivated or activated at any time the Sirius

EQ-G mount is receiving power. In order to deactivate tracking,

simply press and hold the Guide button then press the Slow

button on the controller. Pressing the same button combination

will reactivate tracking at the default (sidereal) rate.

There are three tracking rates used by the dual-axis controller:

Sidereal rate tracking is the default tracking rate for the Sirius

EQ-G mount. Celestial objects are tracked using this rate

which is equivalent to the rate of the Earth’s rotation.

Solar rate tracking is used to track the Sun over a long period

of time. Solar rate tracking is activated by pressing and holding

the Slow speed button, then the Right directional button.

Warning: Never look directly at the Sun through your tele-

scope or its finder scope, even for an instant, without a

professionally made solar filter that completely covers the

front aperture of the instrument, or permanent eye dam-

age could result. Young children should use this telescope

only with adult supervision.

Lunar rate tracking is used to track the Moon at its rate of

apparent motion across the sky. Lunar rate tracking is activat-

ed by pressing and holding the Slow button, then the Down

directional button.

Note: Solar and Lunar tracking rates can only be used when

the Sirius EQ-G has tracking activated. If tracking is deactivat-

ed, you must first activate tracking by holding the Guide button

then pressing the Slow button.

Setting the Slewing Speed

In order to conveniently center an object in your telescope’s

finderscope or eyepiece, you can set the speed rate at which

the motors rotate the telescope when the directional buttons

are pressed. The three speed buttons located near the top of

the hand controller are used to set the slewing rates of the

mount.

The slewing speed buttons each have two different speeds

assigned to them. The slewing speed that is employed is

dependent on whether or not the dual-axis controller has track-

ing activated or deactivated (by holding the Guide button then

pressing the Slow button).

With tracking activated, the Guide button will slew the Sirius

EQ-G mount at a very slow speed equals to 1.5x sidereal rate.

This speed rate will generally be used to guide a telescope

while imaging with a camera. You can also change the Guide

button speed rate to be slightly faster or slower (see “Setting

the Guiding Speed”). If tracking is deactivated, pressing the

Guide button will set the Sirius EQ-G to slew at 32x sidereal

rate; this speed is too fast for guiding during imaging.

By pressing the Slow button with tracking activated, the Sirius

EQ-G will slew at 4x sidereal rate. With tracking deactivated,

pressing the Slow button will set the Sirius EQ-G mount to

slew at 64x sidereal rate.

With tracking activated, the Fast button will set the Sirius EQ-

G mount to slew at 8x sidereal rate. If tracking is not activated,

pressing the Fast button will set the Sirius EQ-G to slew at

800x sidereal rate; this is a very fast speed that can be used to

slew the mount from object to object across the sky.

Changing the Guiding Speed

The dual-axis hand controller provides 4 different guiding

speed settings: 2x, 1.75x, 1.5x (default), and 1.25x sidereal

rate. If you change the guiding speed from the default setting

of 1.5x sidereal rate, the controller will guide at the chosen

speed until another guiding speed is selected.

In order to set the guiding speed of your Sirius EQ-G, use the

following button combinations:

 •2xsiderealrate: HoldtheFast button, then press

the Up directional button.

 •1.75xsiderealrate: HoldtheFast button, then press

the Left directional button.

 •1.5xsiderealrate: HoldtheFast button, then press

the Right directional button.

 •1.25xsiderealrate: HoldtheFast button, then press

the Down directional button.

Reversing the Directional Buttons

Celestial objects appear to move through the sky differently

when viewed through telescopes and/or accessories of dif-

ferent designs. For example, if an object viewed through a

refractor appears to migrate towards the left-hand side of an

eyepiece’s field of view, it will appear to migrate towards the

right-hand side of an eyepiece’s field of view in a reflector

telescope.

In order to make viewing and tracking objects convenient,

regardless of telescope design, the dual-axis controller fea-

tures a “reverse” function which reverses the direction of the

hand controller’s directional buttons. This way you can match

the directional button to the way the object actually moves in

the telescope eyepiece.

To reverse the direction of the Left and Right directional but-

tons, press and hold the Slow speed button then press the

Left directional button. To reverse the direction of the Up and

Down directional buttons, press and hold the Slow button

then press the Up directional button.

Once you have reversed the directional buttons, the dual-axis

controller will save the reversed settings until it they are man-

ually changed again. Turning the power off will not affect the

directional button setting last entered.

Northern or Southern Hemisphere operation

The dual-axis hand controller is capable of operating in either

Northern or Southern Hemisphere viewing locations. The sys-

tem is set up for Northern Hemisphere locations by default, so

if you are viewing from a Northern Hemisphere location, it is

not necessary to make any setting changes.

For the dual-axis controller to properly track celestial objects

in the Southern Hemisphere, press and hold the Down direc-

tional button and then press the Set button while powering

on the mount. Release the Set button after the mount has

successfully powered on and the Guide button begins flash-

ing. The controller will now operate properly in the Southern

Hemisphere. You can switch back to Northern Hemisphere

mode by using the same button combination. As long as the

controller is operating in Southern Hemisphere mode, the Set

button will illuminate.

Power Conservation

In the interest of conserving the amount of power drawn by the

Sirius EQ-G mount, the Dec. motor will enter a “sleep” mode

if left idle for a period of 15 seconds. In “sleep” mode, the Dec.

motor stops completely and the amount of used power drops

by about 40%. To reactivate the Dec. motor, press the Up or

Down directional button.

Upgrading your Sirius EQ-G

While the dual-axis hand controller provides many useful

functions such as celestial object tracking and motorized

motion control, there is a GoTo hand controller for the Sirius

EQ-G available from Orion. The features and functions of the

GoTo hand controller are explained in the following section. If

you are interested in upgrading your Sirius EQ-G to a GoTo

system, call our Customer Service department at 800-676-

1343 or visit our website at www.OrionTelescopes.com for

more information.

8. The Sirius EQ-G GoTo

Hand Controller

The Sirius EQ-G mount equipped with the GoTo hand control-

ler provide easy, computerized location of thousands of night

sky objects such as planets, nebulae, star clusters, galaxies,

and more for viewing through your telescope. The GoTo hand

controller and internal dual-axis motors allow you to automati-

cally point your telescope at a specific object, or tour the skies

with pushbutton simplicity. The user-friendly menu allows

automatic slewing to over 13,400 objects. Even inexperienced

astronomers will find themselves quickly mastering the vari-

ety of features the GoTo hand controller offers in just a few

observing sessions.

Attaching the GoTo Hand Controller

The Sirius EQ-G GoTo hand controller comes with two cables;

one for usage with the Sirius EQ-G mount, while the other is

for use with the Atlas EQ-G mount. After installation, you will

have one of these cables left over. Feel free to discard this

cable, as it will not be needed.

The hand controller cable for the Sirius EQ-G has modular

connectors (RJ-45) on both ends. Plug the modular connector

on one end of the cable into the hand controller jack (Figure

10), and plug the modular connector on the other end of the

cable into the mount’s controller jack (Figure 11). Push the

connectors into the jacks until they click into place.

The smaller modular jack on the hand controller (Figure 10)

is used for RS-232 communications between the Sirius EQ-G

mount and a computer equipped with astronomy software like

Starry Night Pro (see “Linking with a Computer”). The 12V DC

power jack on the hand controller allows independent use of

the GoTo hand controller for users who wish to browse the

object database without connecting to the telescope mount

(Figure 10). The power jack is also used when updating the

firmware in the hand controller (see “Updating the GoTo Hand

Controller’s Firmware”).

The included GoTo hand controller bracket attaches to the

built-in notch in the tripod center support tray. To install the

hand controller bracket, simply line up the tab on the back of

the bracket with the notch in the tripod center support tray and

slide the bracket forward until it clicks into place (Figure 12).

You now have a place to put the GoTo hand controller while

you are viewing.

You can reduce the chances of getting your hand controller

cable tangled during use by installing the included wire clip.

The clip also prevents mechanical strain on the hand control-

ler cable when it is in use. The wire clip is adhesive backed for

easy attachment to any convenient location on the mount.

Powering the Sirius EQ-G Mount

The Sirius EQ-G should be powered by an 11V to 15V DC

power supply (tip positive) capable of producing continuous

current of a minimum 2 amps. We recommend using a por-

table rechargeable battery, like the Dynamo or Dynamo Pro

available from Orion.

If you are using a portable battery like the Orion Dynamo, use

the 12V DC power cable supplied with your mount (male ciga-

rette lighter plug on one end, standard 12V DC power plug on

other end) to connect the battery to the 12V DC power jack on

the mount (Figure 11). Make sure the Dynamo’s power switch

is in the “on” position after connecting. Then, to turn the mount

(and GoTo hand controller) on, simply press the power switch

on the mount so it is in the “on” position.

Note: The power indicator LED on the mount (near the power

switch) will begin to flash when the battery power is low. When

the battery power is extremely low, the LED will flash rapidly.

Recharge or replace the battery as needed.

Functions of the GoTo Hand Controller

There are four main categories of control buttons on the GoTo

hand controller (Figure 13):

1. Mode buttons

2. Directional buttons

3. Scroll buttons

4. Dual Purpose buttons

Mode Buttons

The three mode buttons are located at the top of the con-

troller, directly below the LCD screen. They include the ESC,

ENTER, and SETUP buttons.

The ESC button is used to escape from a certain command or

go back a level in the menu tree.

The ENTER button is used to select the functions and sub-

menus in the menu tree, and to confirm certain functional

operations.

The SETUP button is a “hot key” that takes you to the Setup

Menu.

Directional Buttons

The directional buttons allow the user to have complete motion

Figure 10. Hand controller jacks.

Hand controller

jack

Computer interface

jack

12V DC power jack

Figure 11. The Sirius EQ-G control panel

Autoguider

jack

Power switch

Power indicator light

12V DC power

jack

Hand

controller

jack

Figure 12. Installing the hand controller bracket.

Notch Tripod center

support tray

Hand controller

bracket

control of the Sirius EQ-G mount at almost any step in opera-

tion. These controls are locked out when the mount is slewing

to an object. The directional buttons are very helpful when

initially aligning the mount, centering objects in the eyepiece

field of view, and manual guiding. The directional buttons are

typically used in conjunction with the RATE button. The left

and right directional buttons can also be used to move the text

cursor when entering data into the hand controller.

Scroll Buttons

The up and down scroll buttons allow you to scroll up and

down within the menu tree or selections displayed on the

hand controller screen.

Dual Purpose Buttons

The dual purpose buttons serve two distinct purposes. They

are used for data entry and as quick reference keys.

TOUR button: Takes you on a preset tour of the best night sky

objects visible

RATE button: Changes the speed of the motors when the

directional buttons are pressed. There are 10 speeds to

choose from, with 0 being the slowest and 9 being the fast-

est.

UTILITY button: Provides “hot key” access to the Utility

Functions menu.

USER button: Enter or recall coordinates for up to 25 objects

in the User Defined database.

ID button: Identifies the object the mount is currently pointing

to.

NGC, IC, M, Planet, and Object buttons: Allow direct access

to catalogs and databases of over 13,400 objects.

GoTo Hand Controller

Operation

This section provides a guide for initial setup and alignment of

the Sirius EQ-G mount with the GoTo hand controller.

Initial Setup

1. Perform the polar alignment using the procedure previ-

ously outlined in Section 6 of the instruction manual. A

rough polar alignment will suffice, but an accurate polar

alignment using the polar axis finder scope will increase

tracking accuracy (and pointing accuracy for one-star

alignments).

2. Rotate the telescope tube about the mount’s declination

axis so the tube is parallel with the mount’s R.A. axis (and

the front of the tube is pointed to the sky, not the ground).

Rotate the mount’s R.A. axis so the counterweight shaft is

pointed straight down. The telescope and mount should

now appear as shown in Figure 14. This will be called the

“home” position of the mount.

Note: Once the mount is initially set to its “home” position, the

mount should not be moved manually. Otherwise, the GoTo

Figure 13. The GoTo hand controller.

Display screen

Mode buttons

Directional

buttons

Dual purpose

buttons

Scroll buttons

Figure 14. The telescope and mount in their “home” position

hand controller will lose track of the mount’s position, and the

alignment procedure will need to be performed again. Keep

both the R.A. and Dec. lock levers engaged.

3. Turn on the power switch on the mount

4. The initial screen displayed on the hand controller is the

version screen. Press ENTER to proceed.

5. The hand controller’s LCD screen will show a safe solar

viewing warning message. Press the ESC button to con-

tinue.

Note: The GoTo hand controller’s LCD backlighting will

become dim and the illuminated buttons will turn off if left idle

for 30 seconds. Pressing any button will re-illuminate the hand

controller.

6. Enter your observing site’s longitude and latitude coordi-

nates. First enter the longitude coordinate and hemisphere,

followed by the latitude coordinate and hemisphere. Use

the numerical keypad to enter the digits, and use the left

and right directional buttons to move to the next digit. Use

the scroll buttons to choose W or E (for longitude) and N

or S (for latitude). If you do not know the longitude and

latitude coordinates of your viewing location, consult an

atlas or geographical map of your area. Press ENTER to

confirm your coordinates.

Note: Longitude and latitude coordinates must be entered

in degrees and arcminutes. If your map or atlas gives coor-

dinates in decimal values (i.e. latitude = 36.95 N) you must

convert into degrees and arcminutes (i.e. latitude 36.95 N =

latitude 36°57’ N).

Note: If a mistake is entered into the hand controller during

the initial setup procedure, press the ESC button to go back

to the previous screen.

7. Enter the time zone in which you are observing in hours

(see Appendix D) using the scroll buttons (+ for east of

Prime Meridian, - for west of Prime Meridian) and numeric

keypad. Use the left and right directional buttons to move

to the next digit. Press ENTER to confirm your choice.

8. Enter the date in mm/dd/yyyy format using the numeric

keypad. Use the left and right directional buttons to move

to the next digit. Press ENTER to confirm your choice.

9. Enter your current local time using the 24 hour clock for-

mat (example: 2:00PM = 14:00). Press ENTER to view the

time you entered. If the time is incorrect, press ESC to go

back to the previous screen. If the time is correct, press

ENTER again.

10. If the date entered in step 8 falls between March

and November, the hand controller will ask “DAYLIGHT

SAVING?” on the LCD screen. Use the scroll buttons to

select “YES” or “NO” to indicate if you are currently on

Daylight Savings Time or not, and press ENTER.

11. The hand controller will now display “Begin Alignment?”

Press 1 or ENTER to start the alignment procedure. Press

2 or ESC to skip the alignment and exit to the Main Menu.

You are now ready to begin the alignment procedure.

Alignment

In order for the GoTo hand controller to accurately locate and

point to objects in the sky, it must first be aligned on known

positions (stars). With the supplied information, the controller

can replicate a model of the sky and the movements of astro-

nomical objects.

There are three ways to align depending on your demand for

accuracy. If you are using the GoTo controller for the first time,

we recommend you begin with the three-star alignment. In

most cases, a three-star alignment produces the most accu-

rate alignment among the three methods. The description

below will lead you through a step-by-step procedure on how

to perform the three-star alignment.

Note: Before performing any of the alignment methods, be

sure your finderscope is well aligned with the telescope tube.

Three-Star Alignment

1. From the alignment screen, select “3-Star Align” using the

scroll buttons. Press ENTER to confirm your choice.

2. The hand controller will provide a list of stars available in

your current sky for you to choose as the first alignment

star. Choose a star you are familiar with using the scroll

buttons. Press ENTER to confirm your choice. The mount

will start slewing the telescope towards the chosen object.

When the telescope stops slewing, adjust its position

using the controller’s directional buttons until the chosen

star is centered on the crosshairs of the finderscope. Now

look in the eyepiece and adjust the position of the tele-

scope (again using the directional buttons) so the chosen

star is centered in the field of view of the eyepiece. Press

ENTER to confirm the star is centered .

Note: The slewing speed can be adjusted by pressing the

RATE button. Choose a desired rate between 0 (slowest) and

9 (fastest).

Note: The hand controller will make a “beep” sound once it

has finished slewing to an object. Do not try to adjust the tele-

scope before you hear the “beep” sound. The controller will

only respond to the ESC button while slewing (which stops

the slewing).

3. The controller will provide a list of stars that can be used

as the second alignment star. Choose a star using the

scroll buttons and press ENTER to confirm your choice.

Repeat the centering procedure for the second alignment

star using the directional buttons and press ENTER to

confirm alignment.

4. The controller will once again provide a list of stars that

can be used as the third alignment star. Choose a star

using the scroll buttons and press ENTER to confirm your

choice. Once again, repeat the centering procedure for the

third alignment star and press ENTER to confirm align-

ment.

5. Once the three alignment stars have been entered and

alignment is completed, the hand controller will display

“Alignment Successful.” Press ENTER to access the Main

Menu. Otherwise, “Alignment Failed” will be displayed, and

the alignment procedure must be performed again. To do

this, turn the mount’s power switch off, then on again.

Two-Star Alignment

Two-star alignment requires only two alignment stars but may

produce lesser pointing accuracy than the three-star align-

ment. The description below will lead you on a step-by-step

procedure on how to perform the two-star alignment.

1. From the alignment screen, select “2-Star Align” using the

scroll buttons. Press ENTER to confirm your choice.

2. The hand controller will provide a list of stars available in

your current sky for you to choose as the first alignment

star. Using the scroll buttons, choose a star you are familiar

with and press ENTER to confirm your choice. The mount

will start slewing the telescope towards the chosen star.

When the telescope stops slewing, adjust its position with

the controller’s directional buttons until the star is centered

on the crosshairs of the finderscope. Now look in the eye-

piece and adjust the position of the telescope (again using

the directional buttons) so the chosen star is centered in

the field of view of the eyepiece. Press ENTER to confirm

the star is centered.

3. The controller will provide a list of stars that can be used as

the second alignment star. Choose a star using the scroll

buttons and press ENTER to confirm your choice. Repeat

the centering procedure for the second alignment star and

press ENTER to confirm alignment.

4. Once the two alignment stars have been entered and

alignment is complete, the hand controller will display

“Alignment Successful.” Press ENTER to access the Main

Menu. Otherwise, “Alignment Failed” will be displayed, and

the alignment procedure must be performed again. To do

this, turn the mount’s power switch off, then on again.

One-Star Alignment

One-star alignment is the simplest and quickest alignment

method, as only one alignment star is required. Due to minimal

data input, however, a one-star alignment will not yield optimal

results unless polar alignment is very accurate, and any cone

error is minimized (see Appendix A). The description below will

lead you on a step-by-step procedure on how to perform the

one-star alignment.

1. From the alignment screen, select “1-Star Align” using the

scroll buttons. Press ENTER to confirm your choice.

2. The hand controller will provide a list of stars available in

your current sky for you to choose as the first alignment

star. Using the scroll buttons, choose a star you are familiar

with and press ENTER to confirm your choice. The mount

will start slewing the telescope towards the chosen star.

When the telescope stops slewing, adjust its position with

the controller’s directional buttons until the star is centered

on the crosshairs of the finderscope. Now look in the eye-

piece and adjust the position of the telescope (again using

the directional buttons) so the chosen star is centered in

the field of view of the eyepiece. Press ENTER to confirm

the star is centered.

3. Once the alignment star has been entered and alignment

is complete, the hand controller will display “Alignment

Successful”. Press ENTER to access the Main Menu.

Tips for Choosing Alignment Stars

If possible, use the following tips when choosing alignment

stars for best pointing accuracy.

One-star alignment: Choose a star close to the Celestial

Equator (Dec close to 0°).

Two-star alignment: Choose two stars on the same side of the

meridian, and at least 3 hours apart in right ascension and

3° apart in declination. If you suspect your polar alignment is

poor, choose two stars that are 20° to 60° apart in declination.

Three-star alignment: For the first two stars, follow the tip above

for two-star alignment. For the third alignment star, choose a

star on the other side of the meridian. The first and third align-

ment stars should have declination coordinates between +30°

and +70° or between -30° and -70°.

Pointing Accuracy Enhancement (PAE)

The three-star alignment should provide excellent pointing

accuracy for visual observation. For other applications, such as

CCD imaging, even better pointing accuracy can be obtained

in a specific region of the sky by use of the Pointing Accuracy

Enhancement (PAE) function. Perform the following procedure

to use the PAE function.

1. Choose a bright star near the area of interest in the night

sky. Consult a planisphere or software program to choose

this bright star, if necessary.

2. Find this star in the hand controller’s object database. This

is easily done by pressing the OBJECT button, which

will take you directly to the Named Star database. Press

ENTER to access the list of named stars. Use the scroll but-

tons to peruse the list, and press ENTER to select the star.

Press ENTER again, and the LCD will ask “View Object?”

Press ENTER to issue a command to the mount to GoTo

the star. If the mount is under the control of a computer

running planetarium software, click on the star to slew the

mount to it.

3. Use the directional buttons (and RATE button) to accurate-

ly center the star in a high-powered eyepiece (10mm or

less focal length).

4. Press the ESC button, then press and hold the ESC but-

ton for 2 seconds. The hand controller LCD will read “Re-

center”, and the name of the chosen bright star will blink

three times. If the GoTo command was sent by a computer

running planetarium software, the LCD will read “Last goto

object” instead of the star’s name.

5. Make sure the chosen star is still centered in the eyepiece,

and press the ENTER button. If you don’t want to record

the star position, press the ESC button to exit the PAE

function.

After the PAE function is performed, the hand controller will

recalculate its model of the sky. The pointing accuracy in the

area of sky around the chosen bright star should now be

improved. To improve pointing accuracy in another region of

the sky, perform the PAE function again, this time choosing a

bright star in the new region of interest.

Note: If the mount is “parked” before it is powered off (see “Utility

Functions”), the star alignments and PAE corrections will remain

stored in the hand controller. As long as the mount is not moved

between usage, the alignment will not need to be performed

again when the mount is subsequently powered on.

Object Catalog

The GoTo hand controller boasts a vast database of over

13,400 object coordinates and information. The database

contains the following catalogs:

Named Star - A list of 212 well-known bright stars.

Solar System - The other 8 planets of our solar system, and

the Moon.

NGC - 7,840 of the brightest deep sky objects from the NGC

2000.0 database (edited by Roger W. Sinnott, copyright by

Sky Publishing Corp., used with permission).

IC - 5,386 objects from the Index Catalog.

Messier - Complete list of all 110 Messier objects. These are

some of the most spectacular objects to view in the night sky.

Caldwell - Complete list of all 109 Caldwell objects.

Double Stars - Includes 55 of the best double stars to view.

Variable Stars - Includes 20 of the most well-known variable

stars.

User Defined - Up to 25 objects can be saved in the User

Defined database (see “Using the User Defined Database”).

Selecting an Object

Once the telescope has been aligned, you can access and

view the variety of different objects in the GoTo hand control-

ler’s database. There are three methods of selecting a celes-

tial object to view.

1. Shortcut Buttons

TOUR: Takes you on a preset tour across the night sky.

The brightest and most beautiful deep-sky objects will auto-

matically be chosen by the hand controller for your viewing

pleasure. Use the scroll buttons to view the different deep-

sky objects that are available for viewing through the tour

function. Choose the desired object by pressing ENTER. The

LCD screen will display the coordinates of the chosen object.

Press ENTER again, and the hand controller will ask “View

Object?” Press ENTER once more to have the telescope slew

to the object.

M, NGC, IC: These shortcut buttons give you direct access to

the most popular celestial catalogs. Use the numeric buttons

to select an object by entering its catalog number. Pressing

ENTER will display its coordinate. Primary information such

as size, magnitude, and constellation are obtained by press-

ing the scroll buttons. Press ENTER again, and the hand

controller will ask “View Object?” Press ENTER once more to

have the telescope slew to the object.

PLANET: This shortcut button takes you straight to the Planets

submenu in the hand controller’s database. Use the scroll but-

tons to scroll through the list of planets (and the Moon) in

our solar system. Press ENTER to display the chosen planet’s

coordinates. Press ENTER again, and the hand controller will

ask “View Object?” Press ENTER once more to have the tele-

scope slew to the object. If the planet you selected is currently

below the horizon, the hand controller will prompt you to make

another choice.

USER: This shortcut button will take you to the database that

you have defined for yourself. You can enter a new location or

recall the objects that have been previously saved (see “Using

the User Defined Database”).

2. Object Button

The OBJECT button takes you to the Objects Catalog, where

you have complete access to all of the celestial objects in the

database. Simply scroll through the object catalogs using the

scroll buttons and choose the catalog of objects you wish to

view. Press ENTER to confirm your choice. Use the scroll

buttons to choose an individual object within the catalog and

press ENTER a second time to display the object’s coordi-

nate. Press ENTER again, and the hand controller will ask

“View Object?” Press ENTER once more to have the tele-

scope slew to the object.

3. Menu

You can also access the Objects Catalog through the Main

Menu. In the Main Menu, scroll down to “Object Catalog”

and press ENTER. Like the OBJECT button, this gives you

complete access to the 13,400 celestial objects in the hand

controller’s database.

Other Functions

The GoTo hand controller is equipped with a variety of addi-

tional functions that allow you to optimize performance and

access other features of the system.

Utility Functions

Utility Functions are useful tools that provide simple, yet

handy, processes to enhance your observing experience.

Show Position: Displays the coordinates (right ascension

and declination) of the location where the telescope is cur-

rently pointing.

Display Time: Displays the local time and local sidereal time.

Park Scope: Moves the telescope to the “home” position. This

allows you to power off the Sirius EQ-G mount while saving

alignment and PEC training data. When subsequently pow-

ered on, the initial setup information must again be entered

(be sure to enter the current time accurately!), but the align-

ment procedure can be skipped.

Inquire Version: Displays the hardware, firmware, and data-

base version of the GoTo hand controller. If the hand controller

is connected to the mount, this will also display the firmware

version of the motor control board. Use the scroll buttons to

view the version numbers.

PEC Training: See Appendix B for information

LCD/LED Tuning: Allows adjustments of the LCD charac-

ter contrast, the LCD backlighting, and the LED backlighting

of the pushbuttons. Use the scroll buttons to select which of

these you wish to adjust. Use the left and right directional but-

tons to increase or decrease the value.

Setup Functions

The Setup functions allow you to change any system variable

or information regarding location, time, date, and alignment.

To access the Setup functions, either press the SETUP button

on the hand controller or scroll to “Setup Mode” from the Main

Menu using the scroll buttons and press ENTER. The different

types of functions available to you are listed below, along with

their respective purposes.

Date: Allows you to change the date entered during the initial

setup.

Time: Allows you to change the current time.

Observing site: Allows you to change the current location

(longitude and latitude) setting.

Daylight Savings: Allows you to change the Daylight Savings

option.

Alignment: Allows you to re-perform the star alignment, (see

“Alignment”).

Set Backlash: This function allows you to insert a value for

each axis to compensate for slewing backlash experienced on

that axis. Backlash is a delay in motorized motion of the mount

due to slack between gears. Backlash is experienced when the

slewing direction is reversed on one or both axes of motion.

For improved pointing accuracy, it is important the backlash

value is set to be equal or greater than the actual amount of

backlash between the gears. The default value for the backlash

compensation is 0° 10’ 0” (0 degrees, 10 arcminutes, 0 arc-

seconds). Use the numeric pushbuttons to enter the desired

backlash compensation value. First set the value for R.A. back-

lash compensation, then press ENTER to set the value for

Dec. Press ENTER again to return to the Setup Menu.

Note: Backlash compensation is only active for computerized

slewing, not for manual slewing with the directional buttons.

Set Tracking:

-Sidereal Rate: Activates tracking at sidereal rate. This is

the default tracking rate.

-Lunar Rate: Activates tracking at lunar rate.

-Solar Rate: Activates tracking at solar rate.

-PEC + Sidereal: Activates sidereal rate tracking with

Periodic Error Correction.

-Stop Tracking: Stops tracking.

Warning: Never look directly at the Sun through your tele-

scope or its finder scope, even for an instant, without a

professionally made solar filter that completely covers the

front aperture of the instrument, or permanent eye dam-

age could result. Young children should use this telescope

only with adult supervision.

Auto Guide Speed: When using an autoguider, this sets the

guiding speed to 1.125x, 1.25X, 1.5X, 1.75X, or 2X sidereal

rate.

Using the User Defined Database

The GoTo hand controller allows you to save up to 25 objects

in the User Defined database. You can save unidentifiable

objects, current comet and/or asteroid positions, or make a

custom list of your favorite objects to view.

Saving an Object to the Database

1. Press the USER button. You can also select “User Defined”

in the Object Catalog menu and then press ENTER.

2. Use the scroll buttons to select “Input Coordi.” and press

ENTER.

3. You can ENTER the object’s location by its R.A. and Dec.

coordinates, or its azimuth and altitude coordinates. Press

1 (RA-Dec) or 2 (AzAlt) to make your selection.

4. The default setting will display the R.A./Dec. or Az/Alt coor-

dinates the telescope is currently pointed to. Therefore, if

the telescope is pointing at the object you wish to save

(i.e. the object is centered in the eyepiece), simply press

ENTER. If the object you wish to save is at another location

in the sky, enter its coordinates using the numeric keypad.

When finished inputting the coordinates, press ENTER.

Note: If the coordinates entered do not exist, the hand con-

troller will not respond when ENTER is pressed. Check the

coordinates for data entry mistakes, and re-enter the correct

coordinates.

5. The hand controller will then ask “Save?” If you do wish

to save the entered object coordinates, press ENTER.

Otherwise, press ESC.

6. The controller will now prompt you to choose a num-

ber between 1 and 25 for your chosen object. Using the

scroll buttons, select a number you wish to represent the

object, then press ENTER. Keep in mind that if the object is

assigned a User Object number that is already in use, the

hand controller will overwrite the previously saved coordi-

nates.

7. The hand controller will now display “View Object?” Press

ENTER to slew the telescope to the object, or press ESC

to exit.

Recalling a User Defined Object

1. Press the USER button. You can also select “User Defined”

in the Object Catalog menu and then press ENTER.

2. Choose “Recall Object” and press ENTER.

3. Select the User Object number representing the object you

wish to view using the scroll buttons. Press ENTER to dis-

play the object’s coordinate. Press ENTER again, and the

hand controller will ask “View Object?” Press ENTER once

more to have the telescope slew to the object. (If a vacant

User Object number is selected, the hand controller will not

respond.)

Note: If the recalled User Object is currently below the horizon,

the controller will display “Below Horizon!! Try another obj.” and

will automatically return to “Recall Object”.

Identifying an Unknown Object

The GoTo hand controller has the ability to identify celestial

objects that are unknown to you. To identify an object the

telescope is pointing at, simply press the ID button. You can

also scroll to “Identify” in the Main Menu and press ENTER

to identify the object. The hand controller will then show a list

containing the close objects in the M, IC, NGC, and Named

Star catalogs and their angular distance from the location

where the telescope is pointed. Use the scroll buttons to view

this list of objects. Press ESC when finished.

Linking with a Computer

The GoTo hand controller can be connected to a computer

via the supplied computer interface cable. Many commercially

available planetarium software programs can utilize this func-

tion and be used to control the Sirus EQ-G mount. Look for

software that is compatible with the Celestron NexStar 5i/8i or

NexStar GPS, like Starry Night Pro. The description below will

lead you through the procedure on how to connect and discon-

nect the Sirius EQ-G to a computer.

1. Align the mount as described previously (see “Alignment”).

2. Connect the supplied computer interface cable to the

smaller modular jack (RJ-11) on the hand controller (Figure

10). Connect the other end of the cable to the COM port of

your computer.

3. In the planetarium software of your choice, choose

“Celestron NexStar 5i” or “Celestron 8/9/11 GPS” for the

driver setup and follow the instructions provided by the pro-

gram to connect the mount and computer through the hand

controller. The mount will be under the full control of your

computer once the connection is successfully established.

4. When finished observing, follow the software’s instructions

to close the computer connection to the hand controller.

See Appendix C for more information on computer interfacing.

Auto Guiding

For astronomical imaging, the Sirius EQ-G mount has a des-

ignated autoguider jack (Figure 11). The pin-outs on the 6 pin

modular jack are SBIG compatible and can be used with most

autoguiders available. Refer to Figure 15.1 when connecting

the autoguider cable to the mount and calibrating the autogu-

ider. Autoguiding speed can be adjusted using the “Auto Guide

Speed” function in the Setup Menu.

Updating the GoTo Hand Controller’s Firmware

From version 3.0 and up, the GoTo hand controller’s firmware

can be updated over the internet. Users can download firm-

ware updates from Orion’s website www.OrionTelescopes.

com.

System Requirements

- GoTo hand controller version 3.0 or greater

- Windows95 or later

- An available RS-232 COM port on the PC

- Computer interface cable (supplied)

- DC power supply (7.5V to 15V @ 100mA or greater output

with 2.1mm tip positive plug)

Preparing the Computer for the Update

1. Create a folder where you will store the files necessary for

the update.

2. Go to the website www.OrionTelescopes.com, and access

the support page for the Sirius EQ-G mount.

3. Download and save the Firmware Loader program to the

folder you have created on your computer. You will need to

download this program only once; after it is saved on your

computer, only the firmware data file is needed for future

updates.

4. Download and save the firmware update date file to the

folder you created. The file will be named OrionVxxxxEQ.

ssf, where xxxx indicates the version number of the firm-

ware.

Updating the GoTo Hand Controller

1. Plug the modular plug end of the computer interface cable

into the middle jack in the hand controller (Figure 10). Plug

the serial connector end of the cable to the COM port on

your PC.

2. Press and hold down the 0 and 8 numerical buttons simul-

taneously, then plug the power supply into the hand con-

troller’s DC power jack. The hand controller will beep and

display “SynScan Update Ver. x.x” on the LCD screen.

3. Run the Firmware Loader program on your computer.

4. Click on the “Browse” box and select the OrionVxxxx.ssf

file location where it was saved previously on your com-

puter.

5. Click on the “Update” button, and the new firmware will

begin loading into the hand controller. The Firmware Loader

will show the progress of the update on your computer

screen. It will usually take approximately 5 minutes for the

new firmware to load into the hand controller. It may take

significantly longer if a serial-to-USB adapter is employed

on your computer.

6. When the download is complete, the Firmware Loader will

display “Update Complete”.

The firmware in the GoTo hand controller has now been updat-

ed. You can click on the “HC. Version” button to confirm the

new version number of the firmware (and possibly the data-

Figure 15.1. Pin diagram for the Atlas EQ-G autoguider jack.

base, but the hardware version will not change with internet

updates).

Note: If the error message “Can not connect to a SynScan

hand control” appears on your computer, check all cable con-

nections. Also, try closing all other computer programs that

might be attempting to use the COM port.

Note: If the error message “Firmware update failed...” appears

on your computer, remove the power plug from the hand con-

troller, and then reconnect it. Now, repeat the firmware update

procedure.

By default, the data communication rate between the GoTo

hand controller and the computer is 115kbps. The RS-232

port on some PCs may not support this high data transfer

rate. If the firmware update procedure fails after a few tries,

try reducing the data transfer rate by pressing the SETUP but-

ton on the hand controller. This will reduce the data transfer

rate to 9.6kbps. The controller’s LCD screen will show “Lo” in

the lower right hand corner to indicate the lower transfer rate

setting. The firmware update procedure remains the same

except it will take much longer for the firmware to load into the

hand controller.

Sirius EQ-G GoTo Hand Controller Menu Tree

9. Specifications

Mount: German equatorial

Tripod: Steel

Weight: 30 lbs.

Counterweight: 11 lbs.

Polar axis latitude adjustment: 10° to 65°

Polar axis finder scope: Included, illuminator built

into mount

Motor drives: Dual-axis, internally

housed

Operation: Nor thern or Southern

hemisphere

Power requirement: 12V DC, 2A (tip positive)

Motor type and resolution: Microstep driven 1.8°

stepper motors

Resolution: 0 . 1 4 4 a r c s e c ( o r

9,024,000 steps/rev)

Gear ratio: 705

#7944 Dual-Axis hand controller

Slew speeds: Guiding speed

32x

64x

800x

Guiding speeds: 2x / 1.75x / 1.5x / 1.25x

sidereal rate

Tracking rates: sidereal, lunar, solar

Tracking mode: R.A. tracking

#7947 GoTo hand controller

Slew speeds: Rate 0 = 1.5x

Rate 1 = 2x

Rate 2 = 8x

Rate 3 = 16x

Rate 4 = 32x

Rate 5 = 64x

Rate 6 = 400x

Rate 7 = 500x

Rate 8 = 600x

Rate 9 = 800x (3.4°/sec)

Autoguiding rates: 2x / 1.75x / 1.5x / 1.25x

sidereal rate

Tracking rates: Sidereal (default), lunar,

solar, PEC + sidereal

Tracking modes: R.A. tracking

Alignment method: One-star alignment, two-

star alignment, three-star

alignment

Database: Complete M, NGC, and

IC catalogs, 25 user-

defined objects

Total 13,436 objects

Pointing accuracy: Up to 1 arcminute with

cone error calibration, up

to 15 arcminutes without

cone error calibration.

This device complies with Part 15 of the FCC Rules. Operation

is subject to the following two conditions: (1) this device nay

not cause harmful interference, and (2) this device must

accept any interference received, including interference that

may cause undesired operation.

Changes of modifications not expressly approved by the party

responsible for compliance could void the user’s authority to

operate the equipment.

Note: This equipment has been tested and found to comply

with the limits for a Class B digital device, pursuant to Part

15 of the FCC Rules. These limits are designed to provide

reasonable protection against harmful interference in a resi-

dential installation. This equipment generates, uses and can

radiate radio frequency energy and, if not installed and used in

accordance with the instructions, may cause harmful interfer-

ence to radio communications. However, there is no guarantee

that interference will no occur in a particular installation. If

this equipment does cause harmful interference to radio or

television reception, which can be determined by turning the

equipment off and on, the user is encouraged to try to correct

the interference by one or more of the following measures:

-Reorient or relocate the receiving antenna.

-Increase the separation between the equipment and

receiver.

-Connect the equipment into an output on a circuit different

from that to which the receiver in connected.

-Consult the dealer or an experienced radio/TV technician

for help.

A shielded cable must be used when connecting a peripheral

to the serial ports.

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Orion Sirius EQ?G User manual

Brand: Orion

Model: Sirius EQ?G

Category: Telescopes

Type: User manual

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Orion Sirius EQ?G User manual

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